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<ri:Resource created="2021-10-06T12:07:18Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>8um Cores in NGC 891, NGC 3628 and IC 5052</title><shortName>J/ApJ/895/71</shortName><identifier>ivo://CDS.VizieR/J/ApJ/895/71</identifier><altIdentifier>doi:10.26093/cds/vizier.18950071</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Elmegreen B.G.</name></creator><creator><name>Elmegreen D.M.</name></creator><date role="Updated">2022-03-10T07:10:13Z</date><date role="Created">2021-10-06T12:07:18Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>galaxies</subject><subject>star-forming-regions</subject><subject>infrared-photometry</subject><description>To study the vertical distribution of the earliest stages of star formation in galaxies, three edge-on spirals, NGC891, NGC3628, and IC5052, observed by the Spitzer Space Telescope InfraRed Array Camera (IRAC) were examined for compact 8{mu}m cores using an unsharp mask technique; 173, 267, and 60 cores were distinguished, respectively. Color-color distributions suggest a mixture of polycyclic aromatic hydrocarbons and highly extincted photospheric emission from young stars. The average V-band extinction is ~20mag, equally divided between foreground and core. IRAC magnitudes for the clumps are converted to stellar masses assuming an age of 1Myr, which is about equal to the ratio of the total core mass to the star formation rate in each galaxy. The extinction and stellar mass suggest an intrinsic core radius of ~18pc for 5% star formation efficiency. The half-thickness of the disk of 8{mu}m cores is 105pc for NGC891 and 74pc for IC5052, varying with radius by a factor of ~2. For NGC3628, which is interacting, the half-thickness is 438pc, but even with this interaction, the 8{mu}m disk is remarkably flat, suggesting vertical stability. Small-scale structures like shingles or spirals are seen in the core positions. Very few of the 8{mu}m cores have optical counterparts.</description><source format="bibcode">2020ApJ...895...71E</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/895/71</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/VII/74">VII/74 : Atlas of Peculiar Galaxies (Arp 1966)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/642/158">J/ApJ/642/158 : IRAC flux densities in IC2163 and NGC2207 (Elmegreen+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/669/493">J/ApJ/669/493 : Spitzer/Chandra YSOs in Serpens cloud core (Winston+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/688/237">J/ApJ/688/237 : Disk corrugations in IC 2233 (Matthews+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/135/693">J/AJ/135/693 : X-ray and IR sources in RCW 108 (Wolk+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/184/18">J/ApJS/184/18 : Spitzer survey of young stellar clusters (Gutermuth+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/140/266">J/AJ/140/266 : NGC 1333 X-ray luminous YSOs properties (Winston+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/527/A109">J/A+A/527/A109 : Dust and PAH emission SEDs of disk galaxies (Popescu+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/767/36">J/ApJ/767/36 : APEX observations of HOPS protostars (Stutz+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/146/86">J/AJ/146/86 : Cosmicflows-2 catalog (Tully+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/565/A4">J/A+A/565/A4 : NGC 891 70-500um images (Hughes+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/862/25">J/ApJ/862/25 : H{alpha}&amp;UV emission scale heights for edge-on gal. (Jo+,2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/245/14">J/ApJS/245/14 : 8um cores in spiral arms of nearby galaxies (Elmegreen+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/882/5">J/ApJ/882/5 : ALMA data 5 luminous &amp; ultraluminous IR gal. 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